18 research outputs found
The redshifts of quasars
It has been shown that no correlation exists between the
inferred ejection velocities of quasar absorption lines and the
intrinsic continuum flux. In the absence of a net force on the
absorbing clouds this disproves intrinsic models which rely on
radiative acceleration for the production of these lines.It has also been shown that there is a statistically significant
excess of quasar alignments over that expected at a specific
deviation (four arc - seconds) of the central object from the line
defined by the outlying members. The narrowness of this peak makes
it difficult to explain as the product of simple quasar
clustering.Observation at high spectral resolution om two quasars lying in
such alignments has shown no significant deviations of the
absorption line distribution from the norm. Assuming that this is
true for all such objects and that a significant proportion of the
quasar redshift is gravitational then the observed upper limits on
the rate of change of absorption line redshifts has enabled lower
bounds to be placed upon the central mass. The derived masses are
very large and apparently in conflict with galactic stability
arguments.Number / magnitude distributions have been determined for two
samples of quasar candidates which were previously uncalibrated
Mass transport in galaxy discs limits black hole growth to sub-Eddington rates
Super-massive black holes (SMBHs) observed to have masses of at , Gyr after the Big Bang, are
thought to have been seeded by massive black holes which formed before growing
concurrently with the formation of their host galaxies. We model analytically
the idealised growth of seed black holes, fed through gas inflow from growing
proto-galaxy discs. The inflow depends on the disc gravitational stability and
thus varies with black hole and disc mass. We find that for a typical host
halo, the efficiency of angular momentum transport, as parametrised by the disc
viscosity, is the limiting factor in determining the inflow rate and the black
hole accretion rate. For our fiducial case we find an upper black hole mass
estimate of at .
Only in the extreme case of M haloes at produces
SMBH masses of M. However, the number density of such
haloes is many orders of magnitude below the estimated 1 Gpc of SMBHs at
, indicating that viscosity driven accretion is too inefficient to feed
the growth of seeds into SMBHs by . We demonstrate that major mergers are capable of resolving the
apparent discrepancy in black hole mass at , with some dependence on the
exact choice of orbital parameters of the merger.Comment: 13 pages, 9 figures, accepted for publicatio
The prospect of artificial intelligence to personalize assisted reproductive technology
The Department of Metabolism, Digestion, and Reproduction is funded by grants from the MRC and NIHR. S.H. is supported by the UKRI CDT in AI for Healthcare http://ai4health.io (EP/S023283/1). A.A. is supported by an NIHR Clinician Scientist Award (CS-2018-18-ST2-002). M.V. and K.T.A. are supported by the EPSRC (EP/T017856/1). W.S.D. is supported by an NIHR Senior Investigator Award (NIHR202371).Infertility affects 1-in-6 couples, with repeated intensive cycles of assisted reproductive technology (ART) required by many to achieve a desired live birth. In ART, typically, clinicians and laboratory staff consider patient characteristics, previous treatment responses, and ongoing monitoring to determine treatment decisions. However, the reproducibility, weighting, and interpretation of these characteristics are contentious, and highly operator-dependent, resulting in considerable reliance on clinical experience. Artificial intelligence (AI) is ideally suited to handle, process, and analyze large, dynamic, temporal datasets with multiple intermediary outcomes that are generated during an ART cycle. Here, we review how AI has demonstrated potential for optimization and personalization of key steps in a reproducible manner, including: drug selection and dosing, cycle monitoring, induction of oocyte maturation, and selection of the most competent gametes and embryos, to improve the overall efficacy and safety of ART.Peer reviewe
Optimization of a parallel permutation testing function for the SPRINT R package
The statistical language R and its Bioconductor package are favoured by many biostatisticians for processing microarray data. The amount of data produced by some analyses has reached the limits of many common bioinformatics computing infrastructures. High Performance Computing systems offer a solution to this issue. The Simple Parallel R Interface (SPRINT) is a package that provides biostatisticians with easy access to High Performance Computing systems and allows the addition of parallelized functions to R. Previous work has established that the SPRINT implementation of an R permutation testing function has close to optimal scaling on up to 512 processors on a supercomputer. Access to supercomputers, however, is not always possible, and so the work presented here compares the performance of the SPRINT implementation on a supercomputer with benchmarks on a range of platforms including cloud resources and a common desktop machine with multiprocessing capabilities
FireGrid: Integrated emergency response and fire safety engineering for the future built environment
FireGrid is researching the development and
integration of modelling, sensors, Grid, HPC,
and C/C technologies. It will stimulate further
research, in new safety systems and strategies, in
new sensor technologies, in improved modelling
techniques and in Grid technologies and
operation.
By integrating previously uncoupled tools,
FireGrid will allow true performance-based
design for the built environment. It will
introduce a new emergency response paradigm,
using scenarios planned and stored in advance in
conjunction with super-real-time simulation.
Deployment of FireGrid will reduce costs and
save lives